An astrophysicist-artist's conception of a hypervelocity star speeding away from the visible part of a spiral galaxy like our Milky Way and into the invisible halo of mysterious "dark matter" that surrounds the galaxy's visible portions. University of Utah researcher Zheng Zheng and colleagues in the U.S. and China discovered the closest bright hypervelocity star yet found.

Ben Bromley, University of Utah

A University of Utah-led team discovered a “hypervelocity star” that is the closest, second brightest, and among the largest of 20 found so far. Speeding at more than 1 million mph (1.6 million km/h), the star may provide clues about the supermassive black hole at the center of our Milky Way and the halo of mysterious “dark matter” surrounding the galaxy, astronomers say.

“The hypervelocity star tells us a lot about our galaxy, especially its center and the dark matter halo,” said Zheng Zheng from the University of Utah in Salt Lake City.

“We can’t see the dark matter halo, but its gravity acts on the star,” Zheng said. “We gain insight from the star’s trajectory and velocity, which are affected by gravity from different parts of our galaxy.”

In the past decade, astronomers have found about 20 of these odd stars. Hypervelocity stars appear to be remaining pairs of binary stars that once orbited each other and got too close to the supermassive black hole at the galaxy’s center. Intense gravity from the black hole, which has the mass of 4 million Suns, captures one star so it orbits the hole closely and slingshots the other on a trajectory headed beyond the galaxy.

Zheng and his colleagues discovered the new hypervelocity star while conducting other research into stars with the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) located at the Xinglong Observing Station of the National Astronomical Observatories of China, about 110 miles (180 kilometers) northeast of Beijing. LAMOST boasts a 13.1-foot-wide (4 meters) aperture and houses 4,000 optical fibers, which capture “spectra” or light-wavelength readings from as many as 4,000 stars at once. A star’s spectrum reveals information about its velocity, temperature, luminosity, and size.

LAMOST’s main purpose is to study the distribution of stars in the Milky Way, and thus the galaxy’s structure. The new hypervelocity star — named LAMOST-HVS1 — stood out because its speed is almost three times the usual star’s 500,000-mph (800,000km) pace through space — 1.4 million mph (2.2 million km/h) relative to our solar system. Its speed is about 1.1 million mph (1.8 million km/h) relative to the speed of the center of the Milky Way.

Despite being the closest hypervelocity star, it nonetheless is 249 quadrillion miles (400 quadrillion km) from Earth.

“If you’re looking at a herd of cows, and one starts going 60 mph [100 km/h], that’s telling you something important,” said Ben Bromley from the University of Utah. “You may not know at first what that is. But for hypervelocity stars, one of their mysteries is where they come from — and the massive black hole in our galaxy is implicated.”

The down-low on a fast and loose star
A cluster of known hypervelocity stars, including the new one, is located above the disk of our Milky Way Galaxy, and their distribution in the sky suggests they originated near the galaxy’s center, Zheng said.

The diameter of the visible part of our spiral-shaped galaxy is at least 100,000 light-years. Zheng said that when the halo of dark matter is added, the estimated diameter is roughly 1 million light-years.

Scientists know dark matter halos surround galaxies because of the way their gravity affects the motion of a galaxy’s visible stars and gas clouds. Researchers say only about 5 percent of the universe is made of visible matter, 27 percent is invisible and yet-unidentified dark matter, and 68 percent is even more mysterious dark energy, responsible for accelerating the expansion of the universe. By traveling through the dark matter halo, the new hypervelocity star’s speed and trajectory can reveal something about the mysterious halo.

Our solar system is roughly 26,000 light-years from the center of the galaxy — more than halfway out from the center of the visible disk.

By comparison, the new hypervelocity star is about 62,000 light-years from the galactic center, beyond as well as above the galaxy’s visible disk. It is about 42,400 light-years from Earth.

As far as that is, the star has a magnitude of about 13, or 630 times fainter than stars that barely can be seen with the naked eye. It nevertheless “is the nearest, second brightest, and one of the three most massive hypervelocity stars discovered so far,” Zheng said.

It is nine times more massive than our Sun, which makes it very similar to another hypervelocity star known as HE 0437-5439, discovered in 2005, and both are smaller than HD 271791, which was discovered in 2008 and is 11 times more massive than the Sun. As seen from Earth, only HD 271791 is brighter than LAMOST-HVS1, Zheng said.

The newly discovered hypervelocity star also outshines our Sun. It is four times hotter and about 3,400 times brighter (if viewed from the same distance). But compared with our 4.6-billion-year-old Sun, the newly discovered LAMOST-HVS1 is a youngster born only 32 million years ago, based on its speed and position, Zheng said.

Is there any chance that the supermassive black hole might hurl a hypervelocity star in Earth’s direction one day? Not really, Zheng said. First, astrophysicists estimate only one hypervelocity star is launched every 100,000 years. Second, possible trajectories of stars near the supermassive black hole don’t forebode any danger should any of them become a hypervelocity star in the future.